Pulsar Alignment due to Radiation Reaction Torque

dc.contributor.advisorWetro, Legesse (PhD)
dc.contributor.authorMohammed, Endris
dc.date.accessioned2018-06-22T05:55:06Z
dc.date.accessioned2023-11-09T11:23:26Z
dc.date.available2018-06-22T05:55:06Z
dc.date.available2023-11-09T11:23:26Z
dc.date.issued2010-07
dc.description.abstractWe calculate the time of alignment of the magnetic dipole moment with the axis of rotation. For alignment we take into acount the electromagnetic torque acting on the magnetic dipole moment, the frictional torque between the crust and the core and gravitational effects. The anomalous electromagnetic torque, usually neglected in the a rigid star model, here plays a crucial role for the alignment of the magnetic dipoleen_US
dc.identifier.urihttp://10.90.10.223:4000/handle/123456789/2844
dc.language.isoenen_US
dc.publisherAddis Ababa Universityen_US
dc.subjectRadiation Reaction Torqueen_US
dc.titlePulsar Alignment due to Radiation Reaction Torqueen_US
dc.typeThesisen_US

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